Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-25T20:48:15.780Z Has data issue: false hasContentIssue false
  • English
  • Français

Observations of the J = 6 to 5 Line of OCS in SGR B2

Published online by Cambridge University Press:  14 August 2015

Kenji Akabane ,
Masaki Morimoto ,
Kiyoshi Nagane  and
Norio Kaifu
Kenji Akabane
Affiliation:
Tokyo Astronomical Observatory, Tokyo, Japan
Masaki Morimoto
Affiliation:
Tokyo Astronomical Observatory, Tokyo, Japan
Kiyoshi Nagane
Affiliation:
Tokyo Astronomical Observatory, Tokyo, Japan
Norio Kaifu
Affiliation:
University of Tokyo, Tokyo, Japan

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The J = 6 to 5 line of OCS at 72.9768 GHz was detected in Sgr B2 with antenna temperature 0.3 K, velocity + 62 km s-1, and velocity half width of ∼ 25 km s-1.

Type
Part 5: The Galactic Center
Information
Symposium - International Astronomical Union , Volume 60: Galactic Radio Astronomy , 1974 , pp. 537 - 538
Copyright
Copyright © Reidel 1974 

References

Jefferts, K. B., Penzias, A. A., Wilson, R. W., and Solomon, P. M.: 1971, Astrophys. J. Letters 168, L111.Google Scholar